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761.
建立了T尾有限元模型,以及T尾带后机身等不同支持情况的动力学模型,并分别分析了它们的固有频率特性。为了简化计算规模,只进行一般地定性研究,忽略了T尾平尾有攻角、安装角或上反角引起的附加的广义气动力的影响,用偶极子网格法计算了临界颤振速度,并分析了不同的颤振特性。最后,得出后机身的不同支持刚度对T尾的临界颤振速度影响的趋势曲线。本次计算结果为以后的T尾的颤振分析打下了基础,为后机身的刚度分配提供了宝贵的数据支持。 相似文献
762.
763.
基于主动冷却的脉冲爆震火箭发动机燃油加温实验研究 总被引:1,自引:0,他引:1
在不影响脉冲爆震火箭发动机(PDRE)正常工作的前提下,利用燃油来吸收发动机实验模型工作过程中产生的大量废热,使其主动冷却,更重要的是通过对燃油加温来改善雾化、蒸发和掺混质量,以使PDRE工作得更好。本文设计了五种不同尺寸的爆震管同轴管状换热器,通过实验比较了这些换热器实验件的换热效率,并选取了最高效的换热器用于更进一步的PDRE性能实验。实验结果表明,加有换热器的实验件能快速蒸发燃油,从而改善了燃油雾化和掺混效果并且能延长发动机的工作时间。 相似文献
764.
采用对航天器聚合物介质进行非线性电导改性的方法消除或削弱材料的内带电现象,以期达到消除介质脉冲放电对航天器可靠性的威胁的目标.实验研究发现,采用具有非线性电导率特性的粉粒(添加剂)对航天器用PTFE和EP进行改性,该两种复合介质材料均可产生显著的非线性电导特性.而且,该种添加剂可以显著降低PTFE的非线性电导阈值,改变EP的非线性电导特性的陡度,而不会对两种材料的直流电气强度产生显著影响. 相似文献
765.
766.
文章在建立了线性调频步进ISAR回波信号模型的基础上,对线性调频步进雷达ISAR信号特性进行了详细的分析,指出了由径向速度和转动速度所引起的耦合项、一次项和二次项对距离合成高分辨和方位聚焦的影响;给出了线性调频步进雷达ISAR成像的详细步骤,并用仿真论证了文章分析的可靠性。 相似文献
767.
以小型阵风发生装置为研究对象,采用二维热线风速仪,测量了不同工况下的阵风装置流场参数,给出了二维热线仪测量方案和在线角度修正方法,以及阵风幅值和波形稳定性计算方法。结果表明:采用风洞在线角度修正,可以提高二维热线的y向测量精度和测试效率;采用波形相位分析方法,可以满足阵风发生器产生的周期性波形的幅值和流场脉动量分析;阵风幅值与4~15Hz的叶栅摆动频率、8°~30°的叶栅摆动角度、50~100mm的叶栅弦长成正比关系;阵风波形的不稳定性(等相位速度脉动量)与叶栅摆动角度、来流速度有一定的线性关系,在本试验范围内随叶栅摆动角度、来流速度的增加而增加,同时,适当的叶栅摆动频率可以降低叶栅的波形不稳定性。研究结论对阵风发生装置研制及其流场测量具有一定的参考意义。 相似文献
768.
Sharon Kedar Jose Andrade Bruce Banerdt Pierre Delage Matt Golombek Matthias Grott Troy Hudson Aaron Kiely Martin Knapmeyer Brigitte Knapmeyer-Endrun Christian Krause Taichi Kawamura Philippe Lognonne Tom Pike Youyi Ruan Tilman Spohn Nick Teanby Jeroen Tromp James Wookey 《Space Science Reviews》2017,211(1-4):315-337
InSight’s Seismic Experiment for Interior Structure (SEIS) provides a unique and unprecedented opportunity to conduct the first geotechnical survey of the Martian soil by taking advantage of the repeated seismic signals that will be generated by the mole of the Heat Flow and Physical Properties Package (HP3). Knowledge of the elastic properties of the Martian regolith have implications to material strength and can constrain models of water content, and provide context to geological processes and history that have acted on the landing site in western Elysium Planitia. Moreover, it will help to reduce travel-time errors introduced into the analysis of seismic data due to poor knowledge of the shallow subsurface. The challenge faced by the InSight team is to overcome the limited temporal resolution of the sharp hammer signals, which have significantly higher frequency content than the SEIS 100 Hz sampling rate. Fortunately, since the mole propagates at a rate of \(\sim1~\mbox{mm}\) per stroke down to 5 m depth, we anticipate thousands of seismic signals, which will vary very gradually as the mole travels.Using a combination of field measurements and modeling we simulate a seismic data set that mimics the InSight HP3-SEIS scenario, and the resolution of the InSight seismometer data. We demonstrate that the direct signal, and more importantly an anticipated reflected signal from the interface between the bottom of the regolith layer and an underlying lava flow, are likely to be observed both by Insight’s Very Broad Band (VBB) seismometer and Short Period (SP) seismometer. We have outlined several strategies to increase the signal temporal resolution using the multitude of hammer stroke and internal timing information to stack and interpolate multiple signals, and demonstrated that in spite of the low resolution, the key parameters—seismic velocities and regolith depth—can be retrieved with a high degree of confidence. 相似文献
769.
Mihail P. Petkov Steven M. Jones Gerald E. Voecks Kenneth J. Hurst Olivier Grosjean Delphine Faye Guillaume Rioland Cecily M. Sunday Emma M. Bradford William N. Warner Jerami M. Mennella Ned W. Ferraro Manuel Gallegos David M. Soules Philippe Lognonné W. Bruce Banerdt Jeffrey W. Umland 《Space Science Reviews》2018,214(8):112
We report on the development of a passive sorption pump, capable of maintaining high-vacuum conditions in the InSight seismometer throughout the duration of any extended mission. The adsorber material is a novel zeolite-loaded aerogel (ZLA) composite, which consists of fine zeolite particles homogeneously dispersed throughout a porous silica network. The outgassing species within the SEIS evacuated container were analyzed and the outgassing rate was estimated by different methods. The results were used to optimize the ZLA composition to adsorb the outgassing constituents, dominated by water, while minimizing the SEIS bakeout constraints. The InSight ZLA composite additionally facilitated substantial CO2 adsorption capabilities for risk mitigation against external leaks in Mars atmosphere. To comply with the stringent particle requirements, the ZLA getters were packaged in sealed containers, open to the SEIS interior through \(1~\upmu\mbox{m}\)-size pore filters. Results from experimental validation and verification tests of the packaged getters are presented. The pressure forecast based on these data, corroborated by rudimentary in situ pressure measurements, infer SEIS operational pressures not exceeding \(10^{-5}~\mbox{mbar}\) throughout the mission. 相似文献
770.
Paul Morgan Matthias Grott Brigitte Knapmeyer-Endrun Matt Golombek Pierre Delage Philippe Lognonné Sylvain Piqueux Ingrid Daubar Naomi Murdoch Constantinos Charalambous William T. Pike Nils Müller Axel Hagermann Matt Siegler Roy Lichtenheldt Nick Teanby Sharon Kedar 《Space Science Reviews》2018,214(6):104
This article discusses relevant physical properties of the regolith at the Mars InSight landing site as understood prior to landing of the spacecraft. InSight will land in the northern lowland plains of Mars, close to the equator, where the regolith is estimated to be \(\geq3\mbox{--}5~\mbox{m}\) thick. These investigations of physical properties have relied on data collected from Mars orbital measurements, previously collected lander and rover data, results of studies of data and samples from Apollo lunar missions, laboratory measurements on regolith simulants, and theoretical studies. The investigations include changes in properties with depth and temperature. Mechanical properties investigated include density, grain-size distribution, cohesion, and angle of internal friction. Thermophysical properties include thermal inertia, surface emissivity and albedo, thermal conductivity and diffusivity, and specific heat. Regolith elastic properties not only include parameters that control seismic wave velocities in the immediate vicinity of the Insight lander but also coupling of the lander and other potential noise sources to the InSight broadband seismometer. The related properties include Poisson’s ratio, P- and S-wave velocities, Young’s modulus, and seismic attenuation. Finally, mass diffusivity was investigated to estimate gas movements in the regolith driven by atmospheric pressure changes. Physical properties presented here are all to some degree speculative. However, they form a basis for interpretation of the early data to be returned from the InSight mission. 相似文献